17.2 The Relative Schrödinger Equation. Angular Momentum 733
TheΘFunction
After replacement of the last term on the left-hand side of Eq. (17.2-9) by−m^2 and
multiplication byΘ, we obtainsin(θ)d
dθ(
sin(θ)dΘ
dθ)
−m^2 Θ+Ksin^2 (θ)Θ 0 (17.2-22)This equation can be transformed into a famous equation called theassociated Legendre
equationby the change of variables:ycos(θ), P(y)Θ(θ) (17.2-23)We do not discuss the associated Legendre equation, but give its solutions in Appendix F.
The solutions are calledassociated Legendre functionsand are derivatives of polyno-
mials known asLegendre polynomials.The equation is named for Adrien-Marie
Legendre, 1752–1833, a famous French
mathematician who solved the equation. For a solution of the associated Legendre equation to exist that obeys the relevant
boundary conditions, it turns out that the constantKmust be equal tol(l+1) wherel
is a positive integer at least as large as the magnitude ofm. There is one solution for
each set of values of the two quantum numberslandm:
Θ(θ)Θlm(θ) (17.2-24)Since the equation containsm^2 , the solutions are the same for a given value ofmand
its negative:Θlm(θ)Θl,−m(θ) (17.2-25)where we insert a comma to avoid confusing two subscripts having valuesland−m
with a single subscript having a valuel−m.
If we choose the complexΦfunctions, theYfunctions are calledspherical harmonic
functions.YYlm(θ,φ)Θlm(θ)Φm(φ) (17.2-26)Table 17.1 gives the normalized spherical harmonic functions forl0,l1, and
l2. Additional functions can be derived from formulas in Appendix F.Angular Momentum Values
The spherical harmonic functions,Ylm(θ,φ), are eigenfunctions of̂L^2 with eigenvalue
h ̄^2 K, as in Eq. (17.2-6).̂L^2 Ylm̂L^2 ΘlmΦmh ̄^2 l(l+1)ΘlmΦm (l0, 1, 2,...) (17.2-27)The square of the angular momentum can take on any of the valuesL^2 0, 2h ̄^2 ,6h ̄^2 ,12h ̄^2 ,20h ̄^2 ,...,l(l+1)h ̄^2 ,... (17.2-28)The magnitude of the angular momentum can take on any of the valuesL|L|0,
√
2 h ̄,√
6 h ̄,√
12 h ̄,...,R(√
l(l+1))
h ̄,... (17.2-29)